<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2014-04-15T08:59:00Z" status="active" updated="2026-03-04T11:08:16Z" version="1.2" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>AllWISE color  Red (W4) , Green (W2) , Blue (W1) from raw Atlas Images survey collection</title><shortName>allWISE color</shortName><identifier>ivo://CDS/P/allWISE/color</identifier><altIdentifier>10.26093/cds/aladin/35rf-zj</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Boch T.</name></creator><date role="Created">2014-04-15T08:59:00Z</date><date role="Updated">2019-05-20T08:30:00Z</date><contact><name>CDS Helpdesk</name><email>cds-question@unistra.fr</email></contact></curation><content><subject>Sky survey</subject><subject>Infrared astronomy</subject><subject>Near infrared astronomy</subject><description>NASA's Wide-field Infrared Survey Explorer (WISE; Wright et al. 2010) mapped the sky at 3.4, 4.6, 12, and 22 um (W1, W2, W3, W4) in 2010 with an angular resolution of 6.1", 6.4", 6.5", &amp; 12.0" in the four bands. WISE achieved 5\u03c3 point source sensitivities better than 0.08, 0.11, 1 and 6 mJy in unconfused regions on the ecliptic in the four bands. Sensitivity improves toward the ecliptic poles due to denser coverage and lower zodiacal background. The All-Sky Release includes all data taken during the WISE full cryogenic mission phase, 7 January 2010 to 6 August 2010, that were processed with improved calibrations and reduction algorithms.Original acknowledgement for data: This Progressive Survey distribution makes use of data products from the Wide-field Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, and NEOWISE, which is a project of the Jet Propulsion Laboratory/California Institute of Technology. WISE and NEOWISE are funded by the National Aeronautics and Space Administration.</description><source format="bibcode">2010AJ....140.1868W</source><referenceURL>https://alasky.cds.unistra.fr/AllWISE/RGB-W4-W2-W1</referenceURL><type>Survey</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsDerivedFrom</relationshipType><relatedResource>IPAC/NASA - healpixed by CDS</relatedResource></relationship></content><rights rightsURI="https://cds.unistra.fr/aladin-org/licences_aladin.html">This HiPS is distributed under ODbL license by Unistra/CNRS</rights><capability standardID="ivo://ivoa.net/std/hips#hips-1.0"><interface role="std" xsi:type="vs:ParamHTTP"><accessURL use="base">https://alasky.cds.unistra.fr/AllWISE/RGB-W4-W2-W1</accessURL><mirrorURL>https://alaskybis.cds.unistra.fr/AllWISE/RGB-W4-W2-W1</mirrorURL><mirrorURL>https://irsa.ipac.caltech.edu/data/hips/CDS/AllWISE/RGB-W4-W2-W1</mirrorURL><mirrorURL>https://healpix.ias.u-psud.fr/CDS_P_allWISE_color</mirrorURL><mirrorURL>http://skies.esac.esa.int/AllWISEColor</mirrorURL><mirrorURL>https://hips.china-vo.org/m/CDS_P_allWISE_color</mirrorURL></interface></capability><coverage><temporal>55378 55414</temporal><spectral>7.117148108606838e-21 7.212947919930751e-20</spectral><footprint ivo-id="ivo://mocivod">https://alasky.cds.unistra.fr/AllWISE/RGB-W4-W2-W1/Moc.fits</footprint><waveband>Infrared</waveband></coverage></ri:Resource>